M
Mary K. Hudson
Researcher at Dartmouth College
Publications - 188
Citations - 10516
Mary K. Hudson is an academic researcher from Dartmouth College. The author has contributed to research in topics: Van Allen radiation belt & Magnetosphere. The author has an hindex of 49, co-authored 178 publications receiving 9312 citations. Previous affiliations of Mary K. Hudson include University of California, Los Angeles & University of California, Berkeley.
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MHD/particle simulations of radiation belt dynamics
TL;DR: In this article, the authors used global magnetohydrodynamic models of the Earth-Sun system coupled with test particle simulations of the radiation belts, and showed through two examples that such simulations are capable of capturing the outer zone radiation belt configuration at a variety of time scales and through all phases of a geomagnetic storm.
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Linear stability of the H+ ‐ O+ two‐stream interaction in a magnetized plasma
TL;DR: In this paper, the linear stability of the H(+) - O(+) two-stream interactions for parallel propagating wave modes is extended to an analysis of the stability of wave modes that propagate at an angle to the terrestrial magnetic field.
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Magnetospheric cavity modes driven by solar wind dynamic pressure fluctuations
TL;DR: In this paper, the role of solar wind dynamic pressure fluctuations in the generation of magnetospheric ultra-low frequency (ULF) pulsations was investigated using Lyon-Fedder-Mobarry (LFM) simulations.
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Loss-cone-driven ion cyclotron waves in the magnetosphere
TL;DR: In this paper, the authors examined the theoretical properties of linear ion cyclotron waves propagating in the magnetosphere at arbitrary angles to the background magnetic field and found that in some cases the linear wave growth of modes with oblique propagation can dominate that of the parallel propagating electromagnetic IC wave.
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Electromagnetic ion cyclotron waves in the plasma depletion layer
TL;DR: In this article, the theoretical properties of electromagnetic ion cyclotron (EMIC) waves which occur in the plasma depletion layer are presented, assuming a homogeneous plasma with the characteristics which were measured by the AMPTE/CCE satellite at 1450-1501 UT on October 5, 1984.